Wavelet characterization of 2D turbulence and intermittency in magnetized electron plasmas

被引:5
|
作者
Rome, M. [1 ,2 ]
Chen, S. [1 ,3 ]
Maero, G. [1 ,2 ]
机构
[1] Ist Nazl Fis Nucl, Sez Milano, Via Celoria 16, I-20133 Milan, Italy
[2] Univ Milan, Dipartimento Fis, Via Celoria 16, I-20133 Milan, Italy
[3] China Acad Engn Phys, Inst Fluid Phys, Mianyang 621900, Sichuan, Peoples R China
来源
PLASMA SOURCES SCIENCE & TECHNOLOGY | 2016年 / 25卷 / 03期
关键词
non-neutral plasmas; vortex dynamics; fluid turbulence; wavelet analysis; particle-in-cell simulations; HIGHLY-CHARGED IONS; NONNEUTRAL PLASMAS; COHERENT STRUCTURES; PIC CODE; DYNAMICS; RELAXATION; CONFINEMENT; SIMULATION; VORTICITY; MERGER;
D O I
10.1088/0963-0252/25/3/035016
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
A study of the free relaxation of turbulence in a two-dimensional (2D) flow is presented, with a focus on the role of the initial vorticity conditions. Exploiting a well-known analogy with 2D inviscid incompressible fluids, the system investigated here is a magnetized pure electron plasma. The dynamics of this system are simulated by means of a 2D particle-in-cell code, starting from different spiral density (vorticity) distributions. A wavelet multiresolution analysis is adopted, which allows the coherent and incoherent parts of the flow to be separated. Comparison of the turbulent evolution in the different cases is based on the investigation of the time evolution of statistical properties, including the probability distribution functions and structure functions of the vorticity increments. It is also based on an analysis of the enstrophy evolution and its spectrum for the two components. In particular, while the statistical features assess the degree of flow intermittency, spectral analysis allows us not only to estimate the time required to reach a state of fully developed turbulence, but also estimate its dependence on the thickness of the initial spiral density distribution, accurately tracking the dynamics of both the coherent structures and the turbulent background. The results are compared with those relevant to annular initial vorticity distributions.
引用
收藏
页数:15
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